论文标题

光度LSST天文时间序列分类挑战(Propartc)的结果

Results of the Photometric LSST Astronomical Time-series Classification Challenge (PLAsTiCC)

论文作者

Hložek, R., Ponder, K. A., Malz, A. I., Dai, M., Narayan, G., Ishida, E. E. O., Allam Jr, T., Bahmanyar, A., Biswas, R., Galbany, L., Jha, S. W., Jones, D. O., Kessler, R., Lochner, M., Mahabal, A. A., Mandel, K. S., Martínez-Galarza, J. R., McEwen, J. D., Muthukrishna, D., Peiris, H. V., Peters, C. M., Setzer, C. N.

论文摘要

下一代调查,例如Vera C. Rubin天文台的时空和时间(LSST)的传统调查将产生比以前的调查的数量级。为了准备这些数据洪水,我们开发了光度LSST天文序列分类挑战(ParpartC),该竞赛旨在在非代表性训练集的LSST样条件下催化强大分类器在类似于LSST的情况下的发展,用于大型不平衡类别的光度测试集。 Over 1,000 teams participated in PLAsTiCC, which was hosted in the Kaggle data science competition platform between Sep 28, 2018 and Dec 17, 2018, ultimately identifying three winners in February 2019. Participants produced classifiers employing a diverse set of machine learning techniques including hybrid combinations and ensemble averages of a range of approaches, among them boosted decision trees, neural networks, and multi-layer perceptrons.在IA型超新星和Kilonovae上,前三名分类器的出色表现代表了与天文学内部最新技术的重大改进。本文概述了最有希望的方法,并详细评估了他们的结果,突出了下一代Parlityc数据集的分类器开发和仿真需求的未来方向。

Next-generation surveys like the Legacy Survey of Space and Time (LSST) on the Vera C. Rubin Observatory will generate orders of magnitude more discoveries of transients and variable stars than previous surveys. To prepare for this data deluge, we developed the Photometric LSST Astronomical Time-series Classification Challenge (PLAsTiCC), a competition which aimed to catalyze the development of robust classifiers under LSST-like conditions of a non-representative training set for a large photometric test set of imbalanced classes. Over 1,000 teams participated in PLAsTiCC, which was hosted in the Kaggle data science competition platform between Sep 28, 2018 and Dec 17, 2018, ultimately identifying three winners in February 2019. Participants produced classifiers employing a diverse set of machine learning techniques including hybrid combinations and ensemble averages of a range of approaches, among them boosted decision trees, neural networks, and multi-layer perceptrons. The strong performance of the top three classifiers on Type Ia supernovae and kilonovae represent a major improvement over the current state-of-the-art within astronomy. This paper summarizes the most promising methods and evaluates their results in detail, highlighting future directions both for classifier development and simulation needs for a next generation PLAsTiCC data set.

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